A rough-surface thermophysical model for airless planets

Icarus

Volumn 83, Issue 1, 1990, Pages 27-38

  Spencer, John R ^a  

^a UNIVERSITY OF HAWAII   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0002916736     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(90)90004-S     Document Type: Article

References (23)

1. Intermediate scale lunar roughness
2. Reradiation and thermal emission from illuminated craters on the lunar surface
3. Study of radar echos from the Moon at 23 centimeters wavelenght
4. Apollo 11 and 12 closeup photography
5. Backscattering from an undulating surface with applications to radar returns from the Moon
6. An explication of the radiometric method for size and albedo determination
7. Bidirectional reflectance spectroscopy. 3. Correction for macroscopic roughness
8. Recalibration of the photometric/radiometric method of determining asteroid sizes
9. Wavelength dependence of IRAS asteroid diameters and albedos
10. Radiometry and thermal modeling of asteroids
11. Thermal properties of the regolith of asteroid 1 Ceres
12. A refined “standard” thermal model for asteroids based on observations of 1 Ceres and 2 Pallas
13. Roughness of the lunar soil
14. I. Astronomical Photometry at Wavelengths of 8.5, 10.5, and 11.6 μm. II. Infrared Emission from Asteroids at Wavelengths of 8.5, 10.5, and 11.6 μm
15. Infrared observations of asteroids
16. Radiometry of asteroids
17. Mercury's infrared phase effect
18. Mainbelt asteroids: Dual-polarization radar observations
19. The sunlit lunar surface. I. Albedo studies and full Moon temperature distribution
20. Radar scattering laws for the lunar surface
21. Temperatures on the lunar surface
22. Systematic biases in radiometric diameter determinations
23. Directional characteristics of infrared emission from the Moon